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STEREO-A SECCHI Cor1 Coronagraph

ResourceID
spase://NASA/Instrument/STEREO-A/SECCHI/Cor1

Description

The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from
1.4 to 4 R☉.
https://stereo-ssc.nascom.nasa.gov/publications/CMAD/secchi/STEREO_SECCHI_COR1_CMAD_20211206.pdf

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Details

Version:2.7.1

MetadataRightsList

Rights
SchemeURI
https://spdx.org/licenses/
RightsIdentifierScheme
SPDX
RightsIdentifier
CC0-1.0
RightsURI
https://spdx.org/licenses/CC0-1.0.html
RightsName
Creative Commons Zero v1.0 Universal
Note
CC0 1.0 Universal is the Creative Commons license applicable to all publicly available SPASE metadata descriptions

Version:2.7.1

Instrument

ResourceID
spase://NASA/Instrument/STEREO-A/SECCHI/Cor1
NamingAuthority
NASA
ResourceType
Instrument
ResourceHeader
ResourceName
STEREO-A SECCHI Cor1 Coronagraph
ReleaseDate
2026-02-02 13:11:23Z
RevisionHistory
RevisionEvent
ReleaseDate
2023-10-28 00:08:46Z
Note
Only known prior ReleaseDate of the metadata
RevisionEvent
ReleaseDate
2023-11-02 00:08:46
Note
Changed the ResourceID Naming Authority from SMWG to NASA
RevisionEvent
ReleaseDate
2026-02-02 13:11:23Z
Note
Added MetadataRightsList. Added ResourceType and NamingAuthority. Updated to 2.7.1. Changed http to https in top-level schemaLocation attribute. ZCB
Description

The COR1 telescope is the inner coronagraph of the Sun Earth Connection Coronal and Heliospheric Investigation (SECCHI) instrument suite aboard the twin Solar Terrestrial Relations Observatory (STEREO) spacecraft. Like all coronagraphs, COR1 is designed to measure the weak light from the solar corona in the presence of scattered light from the much brighter solar photosphere. It designed to observe the white light corona from
1.4 to 4 R☉.
https://stereo-ssc.nascom.nasa.gov/publications/CMAD/secchi/STEREO_SECCHI_COR1_CMAD_20211206.pdf

Contacts
RolePersonStartDateStopDateNote
1.ProgramScientist
PrincipalInvestigator		spase://SMWG/Person/Charles.N.Arge
2.CoInvestigatorspase://SMWG/Person/O.Chris.St.Cyr
3.CoInvestigatorspase://SMWG/Person/William.T.Thompson
4.CoInvestigatorspase://SMWG/Person/Nat.Gopalswamy
5.CoInvestigatorspase://SMWG/Person/Barbara.J.Thompson
6.CoInvestigatorspase://SMWG/Person/Hong.Xie
PriorIDs
spase://SMWG/Instrument/STEREO-A/SECCHI/Cor1
InstrumentType
Coronograph
InvestigationName
SECCHI
ObservatoryID
spase://SMWG/Observatory/STEREO-A